Contribution of Characteristic X-rays to the Radiation of Solar Flares
โ Scribed by ACTON, LOREN W.
- Book ID
- 109645421
- Publisher
- Nature Publishing Group
- Year
- 1965
- Tongue
- English
- Weight
- 246 KB
- Volume
- 207
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/207737a0
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๐ SIMILAR VOLUMES
The polarization of hard solar X-radiation (> l0 keV) is calculated on the assumption that electrons get a non-isotropic velocity distribution in the initial phase of a flare. The bremsstrahlung generated by nonthermal electrons spiralling around magnetic field lines with discrete pitch angles is co
The problem of producing the hard X-ray burst at the onset of solar flares may be thought of in terms of the problem of producing the non-thermal electrons which emit the X-rays via bremsstrahlung. Electron acceleration to relativistic energies without similar ion acceleration is difficult to achiev